IRAS 05306-7032 , the SIMBAD biblio

IRAS 05306-7032 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.26CEST12:42:39


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Title First 3 Authors
1997A&A...325..585V 62 50 Obscured Asymptotic Giant Branch stars in the Magellanic Clouds. III. New IRAS counterparts. VAN LOON J.T., ZIJLSTRA A.A., WHITELOCK P.A., et al.
1997A&AS..125..419L viz 799 45 Obscured AGB stars in the Magellanic Clouds. I. IRAS candidates. LOUP C., ZIJLSTRA A.A., WATERS L.B.F.M., et al.
2001AJ....122.1844E viz 1826 79 MSX, 2MASS, and the Large Magellanic Cloud: a combined near- and mid-infrared view. EGAN M.P., VAN DYK S.D. and PRICE S.D.
2009AJ....137.3139V viz 15       D               1 1973 42 Variable evolved stars and young stellar objects discovered in the large Magellanic cloud using the SAGE survey. VIJH U.P., MEIXNER M., BABLER B., et al.
2009ApJS..184..172G viz 15       D               1 2912 133 High- and intermediate-mass young stellar objects in the Large Magellanic Cloud. GRUENDL R.A. and CHU Y.-H.
2011A&A...530A..90V viz 15       D               1 1414 46 The optically bright post-AGB population of the LMC. VAN AARLE E., VAN WINCKEL H., LLOYD EVANS T., et al.
2016ApJ...826...44S viz 16       D               1 237 24 The infrared spectral properties of Magellanic carbon stars. SLOAN G.C., KRAEMER K.E., McDONALD I., et al.
2018A&A...609A.114G viz 16       D               408 55 Luminosities and mass-loss rates of Local Group AGB stars and red supergiants. GROENEWEGEN M.A.T. and SLOAN G.C.
2019A&A...626A..92G viz 59       D     X         2 225 ~ 30-micron sources in galaxies with different metallicities. GLADKOWSKI M., SZCZERBA R., SLOAN G.C., et al.
2019ApJ...887...82K viz 17       D               1 263 ~ Stellar pulsation and the production of dust and molecules in galactic carbon stars. KRAEMER K.E., SLOAN G.C., KELLER L.D., et al.
2020A&A...636A..48G viz 17       D               3 970 ~ The VMC Survey. XXXVII. Pulsation periods of dust-enshrouded AGB stars in the Magellanic Clouds. GROENEWEGEN M.A.T., NANNI A., CIONI M.-R.L., et al.

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